Résumé
The Ultra-Fast Flash Observatory (UFFO) pathfinder is a space mission devoted to the measurement of Gamma-Ray Bursts (GRBs), especially their early light curves which will give crucial information on the progenitor stars and central engines of the GRBs. It consists of two instruments: the UFFO Burst Alert & Trigger telescope (UBAT) for the detection of GRB locations and the Slewing Mirror Telescope (SMT) for the UV/optical afterglow observations, upon triggering by UBAT. The UBAT employs a coded-mask γ/X-ray camera with a wide field of view (FOV), and is comprised of three parts: a coded mask, a hopper, and a detector module (DM). The UBAT DM consists of a LYSO scintillator crystal array, multi-anode photo multipliers, and analog and digital readout electronics. We present here the design and fabrication of the UBAT DM, as well as its preliminary test results.
| langue originale | Anglais |
|---|---|
| Pages | 235-238 |
| Nombre de pages | 4 |
| Les DOIs | |
| état | Publié - 1 janv. 2011 |
| Modification externe | Oui |
| Evénement | 32nd International Cosmic Ray Conference, ICRC 2011 - Beijing, Chine Durée: 11 août 2011 → 18 août 2011 |
Une conférence
| Une conférence | 32nd International Cosmic Ray Conference, ICRC 2011 |
|---|---|
| Pays/Territoire | Chine |
| La ville | Beijing |
| période | 11/08/11 → 18/08/11 |
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